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1.
2003年11月20日磁暴主相期间,Cluster卫星正好处在黄昏侧的磁鞘附近.在主相期间磁鞘磁场Bz分量大约为-60 nT,这和ACE卫星观测值基本一致.同时,磁鞘中的离子速度分布对磁鞘中的磁场方向有很强的依赖性.行星际电场Ey在磁鞘中大约是50 mV/m.磁鞘中这些极端的磁场,电场和离子的流动驱动了迄今23个太阳活动周期中最大的磁暴,其Dst指数是-472 nT.Cluster卫星观测发现磁鞘中离子的数密度比较低,这可能是由磁云经过地球时太阳风的低密度造成的.磁鞘中能量范围为1～10 keV的H+,He+和He2+的数密度主要是由磁鞘中太阳风的数密度决定的.同时,对磁鞘中存在大量的1～10 keV氧离子进行了讨论.在极端的南向行星际磁场条件下,磁层顶受到很强的压缩.氧离子可以利用较大的回旋半径,在强压缩的磁层顶和磁鞘对流的共同影响下进入磁鞘.这也表明了磁层对极端行星际条件的一种响应.Cluster卫星在11月20日磁暴事件中的观测研究,对进一步全面认识大磁暴事件有很重要的作用. 相似文献
2.
《地球物理学进展》2015,(3)
为探测掘进前方隐伏的含水构造,预防地质水害,解决煤巷综掘过程中日益突出的"探、掘"矛盾,论文提出和研究电场约束法煤巷综掘探测方法.该方法利用电场同性相斥的原理,使发射电场被约束在一定范围内,达到定方向定距离探测的目的.根据该方法基本原理,建立超前探测有限元仿真模型,开展相应的数值模拟.论文主要从探测基本方法,激发极化程度、异常体的体积大小及巷道内金属体对于超前探测的影响展开模拟研究.结果表明,该方法可以有效探知掘进面前方的含水地质异常,其探测有效距离约为10m.该研究为电场约束法煤巷综掘超前探测方法的实现奠定了理论基础,对综掘超前探测技术的发展具有重要的推动作用. 相似文献
3.
时间域航空电磁系统的探测深度是一项关键技术参数,在系统研制设计和资料解释中都有重要作用.当目标层与围岩电性差异不大或目标层引起的异常响应不明显时,常规的估算探测深度方法不再适用,为克服这种缺陷,本文提出了一种系统探测深度的估算方法,该方法通过模拟电场在均匀半空间模型和层状模型中的扩散过程,记录电场最大幅值在地下的瞬时位置,将系统的探测深度定义为观测到的响应值等于给定的噪声水平时,对应时刻的地下介质中感应电场幅度的最大值对应的深度.论文以我国自主研制的直升机时间域航空电磁系统CHTEM-I为例,根据对不同条件下的计算结果的分析,给出了探测深度与模型电导率、飞行高度和噪声水平之间的关系曲线,并总结出一些能够提高系统探测深度的建议.结果表明半空间模型电导率在0.000295~0.0422S/m范围内,CHTEM-I系统可以在噪声水平与t-0.5成正比条件下达到300m的探测深度.本文方法的估算结果不受模型层厚薄,或目标层与围岩电性差异小等因素影响,因而具有较高的实用性.文中的结论对时间域航空电磁系统设计有理论指导意义,也可用于其它时间域电磁勘探系统探测深度的估算. 相似文献
4.
本文根据ＬＥＯ中等离子体温度低，密度高，德拜长度小的特点，采用薄鞘层近似，计算了离子收集电流；根据电流平衡方程，考虑表面二次电子发射，计算了大型航天器表面在沉降电子流辐照下的充电特性。 相似文献
5.
时间域航空电磁系统的探测深度是一项关键技术参数,在系统研制设计和资料解释中都有重要作用.当目标层与围岩电性差异不大或目标层引起的异常响应不明显时,常规的估算探测深度方法不再适用,为克服这种缺陷,本文提出了一种系统探测深度的估算方法,该方法通过模拟电场在均匀半空间模型和层状模型中的扩散过程,记录电场最大幅值在地下的瞬时位置,将系统的探测深度定义为观测到的响应值等于给定的噪声水平时,对应时刻的地下介质中感应电场幅度的最大值对应的深度.论文以我国自主研制的直升机时间域航空电磁系统CHTEM-I为例,根据对不同条件下的计算结果的分析,给出了探测深度与模型电导率、飞行高度和噪声水平之间的关系曲线,并总结出一些能够提高系统探测深度的建议.结果表明半空间模型电导率在0.000295~0.0422 S/m范围内,CHTEM-I系统可以在噪声水平与t－0.5成正比条件下达到300 m的探测深度.本文方法的估算结果不受模型层厚薄,或目标层与围岩电性差异小等因素影响,因而具有较高的实用性.文中的结论对时间域航空电磁系统设计有理论指导意义,也可用于其它时间域电磁勘探系统探测深度的估算. 相似文献
6.
为了对雷暴云下近地面的电特性进行分析，本文建立了模拟自然尖端所产生的电晕离子演化的一维数值模式。以地面电场为基础，考虑到地面电晕离子的演化，成功地计算了从地面至８００ｍ的空中电场及电荷、电流的时空演变，发现地面电晕离子可解释除雷暴云电荷影响外的空中电场和地面电场的差异，空间电场比地面电场更能反应雷暴电荷所产生的电场。空间电荷层可延伸到８００ｍ的高度上，且电荷密度可高达０．２５ｎＣ／ｍ３，６００ｍ高度上的传导电流密度可达０．１ｎＡ／ｍ２。 相似文献
7.
极盖等离子体云块是极区空间天气重要现象之一,其形成过程是当前重要研究课题.观测表明,日侧磁场重联对应的极区电离层高速流可能对舌状等离子体(TOI)形成"切割"作用,最终形成极盖等离子体云块.伴随磁场重联,同时存在极光粒子沉降,会引起F层等离子体密度的增大,阻碍"切割"效应.本文利用耦合极区电离层模型,模拟研究电场和软电子沉降共同作用下F层等离子体密度的演化.结果表明,在局部电离层电场大于一定数值(80 mV)的情况下,"切割"效应能有效发生.并详细分析了"切割"效应发生时等离子体各参量的演化过程,对"切割"效应的内在物理过程进行了探讨. 相似文献
8.
自20世纪90年代首次探测到410-km间断面上覆低速层以来,全球多个俯冲带和大陆克拉通地区都陆续发现了该低速层结构.对其特性及形成机理的探讨是深部地幔结构、物性和动力学研究的热点问题.本文聚焦于西北太平洋俯冲地区410-km间断面上覆低速层的探测及特性研究上.通过对发生于日本北海道地区两个中等深度地震区域波形资料的分析,利用三重震相波形拟合方法获得了我国东北及日本海西北部下方410-km间断面附近的P波速度结构.速度模型明确显示,410-km间断面上方存在厚~47±14 km,异常值~2%的低速层,横向展布近700 km.结合区域地震层析成像、矿物高温高压物理实验及动力学模拟结果,我们否定了"从下至上"的上涌热物质导致410-km间断面上覆低速层的模型;认为较老且快速俯冲的太平洋板块在地幔过渡带顶部脱水导致硅酸盐矿物的部分熔融,由于熔体密度较大能够稳定存在于410-km间断面之上,从而产生了观测到的横向展布较广的410-km间断面上覆低速层结构. 相似文献
9.
运用双流体MHD方程描述电子和离子的行为, 采用非扰动理论, 把孤子看作经典粒子, 通过推导的赝势(也称Sagdeev势)方程, 结合数值计算来研究惯性区低-β等离子体中动力学Alfvén孤波的特性. 结果表明离子热效应对Alfvén孤波特性的影响不可忽略, 且在惯性区稀疏型孤波和压缩型孤波均存在. 此结论与Freja卫星在极区上空所观测结果吻合很好. Alfvén孤波携带有平行电场, 它对带电粒子的加速有重要作用, 这给极光粒子加速提供了一种可能的物理机制. 相似文献
10.
为对水中目标电磁特性进行数学建模及深度换算,以及对水中目标实施空中探测、定位,将镜像法应用于存在两个分界面的含导电媒质的分层媒质中,在唯一性原理的基础上,推导了空气-海水-海床三层模型下,位于海水中的任意静态电偶极子在源所在媒质区域以外的空间中-空气中的电场、磁场分布的解析表达式,并以单位偶极矩的水平电偶极子为例进行了仿真计算和特征分析.所得解析表达式为后续相关研究提供理论基础,仿真结果和文献对比,表明浅海环境下海水中的静态电偶极子在空气中也可以产生明显的电场、磁场,而且具有明显分布特征,是值得关注的目标信号. 相似文献
11.
Luminescence thermochronometry is sensitive to very low temperatures (below ∼120 °C), and enables the resolution of thermal histories over sub-Quaternary timescales. Here we apply a multi-elevated-temperature post-infrared infrared-stimulated luminescence (MET-pIR-IRSL) measurement protocol to feldspar minerals to extract thermal histories. These thermal histories depend on the thermal stability of the MET signal, and are based on the thermal kinetic parameters extracted from isothermal decay experiments. However, the derived thermal kinetic parameters vary with experimental conditions, specifically with the isothermal holding temperatures (ITL) used. We analyse samples with independently known thermal histories, together with synthetic thermal history samples and samples with unknown thermal histories to test the validity of thermal kinetic parameters obtained from different combinations of isothermal holding data. This approach is tested on feldspars of different mineralogies and lithologies. We find that the temperatures inferred from inverting the data change, depending both on the number and on the highest ITL temperature used for thermal kinetic parameter derivation. Analysed samples validate the MET-pIR-IRSL protocol for extracting thermal histories, and we suggest that four isothermal holding temperatures between 190 and 250 °C are used for appropriate thermal kinetic parameter derivation. 相似文献
12.
We compare different past sea level reconstructions over the 1950–2009 time span using the Empirical Orthogonal Function (EOF) approach. The reconstructions are based on 91 long (up to 60?years) but sparsely distributed tide-gauge records and gridded sea level data from two numerical ocean models over 1958–2007 (the DRAKKAR/NEMO model without data assimilation and the simple ocean data assimilation ocean reanalysis-SODA-) and satellite altimetry data over 1993–2009. We find that the reconstructed global mean sea level computed over the?~60-year-long time span little depends on the input spatial grids. This is unlike the regional variability maps that appear very sensitive to the considered input spatial grids. Using the DRAKKAR/NEMO model, we test the influence of the period covered by the input spatial grids and the number of EOFs modes used to reconstruct sea level. Comparing with tide-gauge records not used in the reconstruction, we determine optimal values for these two parameters. As suggested by previous studies, the longer the time span covered by the spatial grids, the better the fit with unused tide gauges. Comparison of the reconstructed regional trends over 1950–2009 based on the two ocean models and satellite altimetry grids shows good agreement in the tropics and substantial differences in the mid and high latitude regions, and in western boundary current areas as well. The reconstructed spatial variability seems very sensitive to the input spatial information. No clear best case emerges. Thus, using the longest available model-based spatial functions will not necessarily give the most realistic results as it will be much dependent on the quality of the model (and its associated forcing). Altimetry-based reconstructions (with 17-year long input grids) give results somewhat similar to cases with longer model grids. It is likely that better representation of the sea level regional variability by satellite altimetry compensates the shorter input grids length. While waiting for much longer altimetry records, improved past sea level reconstructions may be obtained by averaging an ensemble of different model-based reconstructions, as classically done in climate modelling. Here, we present such a ‘mean’ reconstruction (with associated uncertainty) based on averaging the three individual reconstructions discussed above. 相似文献
13.
W. Kofman 《Surveys in Geophysics》1992,13(6):551-571
The incoherent scatter technique has been applied since 1965 to study the ionosphere and thermosphere in different regions of the Earth. The analysis of the received signal gives access to several ionospheric parameters as a function of height: electron density, electron and ion temperatures and ion velocity. The derivation of these parameters is usually a complicated mathematical procedure that requires a non-linear regression program. A lot of research has been done in the ionospheric and atmospheric science using this technique.In this paper we describe how one derives the ion-neutral collision frequency and the ion composition parameters. It is usually difficult to retrieve these parameters with the incoherent scatter technique; as a result, in the standard data analysis procedure, an ionospheric model is used instead. However the numerical values chosen in the model have an influence on the other derived parameters. For instance the choice of a wrong ion composition leads to erroneous plasma temperatures. It is therefore important to assess by how much the standard procedure deviates from reality. For this reason we compare the ion composition and collision frequency retrieved from a sophisticated analysis scheme with the values that are derived from models under similar geophysical conditions.It also possible to derive from the observed ionospheric parameters the neutral concentrations, temperatures and winds, by using the energy and momentum equations for the ions and the neutrals. In this paper the different methods and the corresponding assumptions involved in the data analysis are discussed. We describe the influence of the frictional heating, of the vertical neutral wind and of the ionospheric perturbations on the derivation of the neutral atmospheric parameters. Our discussion of the processes involved are drawn from results obtained by Chatanika, Sondrestrom and EISCAT radars. 相似文献
14.
在山区进行MT勘探时,用规则网格有限元方法模拟起伏地形会受到限制.本文采用非结构三角网格可以有效地模拟任意二维地质结构,如起伏地形、倾斜岩层和多尺度构造等.正演引入自适应有限元方法,其在网格剖分过程中能根据单元误差自动细化网格,保证了正演结果的精度.将自适应有限元与Occam算法结合,且引用并行处理技术提高正反演计算速度.通过对比两个理论模型,讨论了地形对MT正演响应的影响;其次进行了不同地电模型带地形反演展示了本文算法的正确性和适用性;最后将该方法应用于实测MT数据处理,证明了自适应非结构有限元方法是复杂地形下处理MT数据的有力工具. 相似文献
15.
Simultaneous quantification of epistemic and aleatory uncertainty in GMPEs using Gaussian process regression 总被引：2，自引：2，他引：0
Marcel Hermkes Nicolas M. Kuehn Carsten Riggelsen 《Bulletin of Earthquake Engineering》2014,12(1):449-466
This paper presents a Bayesian non-parametric method based on Gaussian Process (GP) regression to derive ground-motion models for peak-ground parameters and response spectral ordinates. Due to its non-parametric nature there is no need to specify any fixed functional form as in parametric regression models. A GP defines a distribution over functions, which implicitly expresses the uncertainty over the underlying data generating process. An advantage of GP regression is that it is possible to capture the whole uncertainty involved in ground-motion modeling, both in terms of aleatory variability as well as epistemic uncertainty associated with the underlying functional form and data coverage. The distribution over functions is updated in a Bayesian way by computing the posterior distribution of the GP after observing ground-motion data, which in turn can be used to make predictions. The proposed GP regression models is evaluated on a subset of the RESORCE data base for the SIGMA project. The experiments show that GP models have a better generalization error than a simple parametric regression model. A visual assessment of different scenarios demonstrates that the inferred GP models are physically plausible. 相似文献
16.
New results on the information that can be extracted from simulated non-Maxwellian incoherent radar spectra are presented. The cases of a pure ionosphere and of a composite ionosphere typical of a given altitude of the auroral F region are considered. In the case of a pure ionosphere of NO+ or O+ ions it has been shown that the electron temperature and the electron density can be derived from a Maxweilian analysis of radar spectra measured at aspect angles of 0° or 21° respectively; the ion temperature and ion temperature anisotropy can be derived from a non- constraining model such as the ID Raman fitting of a complementary measurement made at an aspect angle larger than 0° for the NO+ ions, or at an aspect angle larger than 21° for the O+ ions. Moreover with such measurements at large aspect angles, the shape of the velocity ion distribution functions can simultaneously be inferred. The case of a composite ionosphere of atomic O+ and molecular NO+ions is a difficult challenge which requires simultaneously a complementary measurement of the electron temperature to provide the ion composition and the electron density from the incoherent radar spectra at a specific aspect angle of 21°; hence, a model dependent routine is necessary to derive the ion temperatures and ion temperature anisotropies. In the case where the electron temperature is not given, a routine which depends on ion distribution models is required first: the better the ion distribution models are, the more accurately derived the plasma parameters will be. In both cases of a composite ionosphere, the 1D Raman fitting can be used to keep a check on the validity of the results provided by the ion distribution model dependent routine. 相似文献
17.
—?Measurements of group velocity are derived from phase-velocity dispersion curves and modeled with global laterally-varying isotropic structure. Maps for both Love and Rayleigh waves are created in the period range 35?s to 175?s. The data set of group-velocity measurements includes over 50,000 minor-arc observations and 5,000 major-arc observations. The errors in the measurements are estimated by an empirical method of comparing pairwise-similar paths, resulting in uncertainties which are 20% to 40% of the size of the typical measurement. The models are determined by least-squares inversion for spherical harmonic maps expanded up to degree 40. This parameterization allows for resolution of structures as small as 500?km. The models explain 70–98% of the variance relative to the Preliminary Reference Earth Model (PREM). For the area of Eurasia, the group-velocity maps from this study are compared with those of Ritzwoller and Levshin (1998). The results of the two studies are in very good agreement, particularly in terms of spatial correlation. The models also agree in amplitude at wavelengths longer than 30?degrees. For shorter wavelengths, the agreement is good only for models at short periods. The global maps are useful for prediction of group arrival times, for revealing tectonic structures, for determination of seismic event locations and source parameters, and as a basis for regional group-velocity studies. 相似文献
18.
快速准确的海啸源模型是近场海啸精确预警的关键.尽管目前还没有办法直接对其进行正演定量计算,但是可以通过多源地震、海啸观测数据进行反演或联合反演推算.不同的海啸源可能导致不同的预警结论,了解不同类型海啸源适用性、评估海啸源特征差异对近场海啸的影响,无论对于海啸预警还是海啸模拟研究尤为重要.本文评估分析了6种不同同震断层模型对2011年3月11日日本东北地震海啸近场数值预报的影响,重点对比分析了有限断层模型与均一滑动场模型对近场海啸产生、传播、淹没特征的影响及各自的误差.研究表明:近场海啸波能量分布主要取决于海啸源分布特征,特别是走向角的差异对海啸能量分布影响较大;有限断层模型对海啸灾害最为严重的39°N以南沿岸地区的最大海啸爬坡高度明显优于均一滑动场模型结果;综合对比DART浮标、GPS浮标及近岸潮位站共32个站次的海啸波幅序列结果发现有限断层模型整体平均绝对/相对误差比均一滑动场模型平均误差要低,其中Fujii海啸源的平均绝对/相对误差最小,分别是0.56m和26.71%.UCSB海啸源的平均绝对/相对误差次之.3个均一滑动场模型中USGSCMT海啸源模拟精度最高.相对于深海、浅海观测站,有限断层模型比均一滑动场模型对近岸观测站计算精度更高.海啸源误差具有显著的方向性,可能与反演所采用的波形数据的代表性有关;谱分析结果表明Fujii海啸源对在12至60min主频波谱的模拟要优于UCSB海啸源.海啸源中很难真实反映海底地震破裂过程,然而通过联合反演海啸波形数据推算海啸源的方法可以快速确定海啸源,并且最大限度的降低地震破裂过程与海啸产生的不确定性带来的误差. 相似文献
19.
Examining the effect of geomorphic characteristics on pool temperatures for native fish habitat management in mountainous stream networks 
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下载免费PDF全文 Stream temperature is a critical habitat parameter for cold‐water fish, many species of which now exist in geographically fragmented populations within the western United States. To assist managers in identifying thermally suitable fish habitat, we used data from 31 pools on streams of the White River National Forest in Colorado, USA to create multiple regression models to predict summer pool temperature metrics related to lethal and sublethal thermal tolerances of fish. We modeled the 7‐day mean of daily maximum pool temperature for the warmest 7 days and the mean temperature of the warmest month, using air temperature and several geomorphic parameters. The strongest predictor variables of these temperature metrics were drainage area, discharge, and residual pool volume. Most previous studies found air temperature to be the strongest predictor variable for pool temperature, but for the mountain streams in this study, variables related to stream flow volume and stream morphology had better predictive power. The models, created from and tested against field data, were able to explain 66% and 51% of the variability in monthly mean and 7‐day mean pool temperatures, respectively, and had prediction errors of less than 2°C. The reach‐scale approach developed here, which includes geomorphically relevant predictors of pool temperature, should be applicable to other mountainous river networks. Copyright © 2016 John Wiley & Sons, Ltd. 相似文献
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The travel time and amplitude of ground-penetrating radar (GPR) waves are closely related to medium parameters such as water content, porosity, and dielectric permittivity. However, conventional estimation methods, which are mostly based on wave velocity, are not suitable for real complex media because of limited resolution. Impedance inversion uses the reflection coefficient of radar waves to directly calculate GPR impedance and other parameters of subsurface media. We construct a 3D multiscale stochastic medium model and use the mixed Gaussian and exponential autocorrelation function to describe the distribution of parameters in real subsurface media. We introduce an elliptical Gaussian function to describe local random anomalies. The tapering function is also introduced to reduce calculation errors caused by the numerical simulation of discrete grids. We derive the impedance inversion workflow and test the calculation precision in complex media. Finally, we use impedance inversion to process GPR field data in a polluted site in Mongolia. The inversion results were constrained using borehole data and validated by resistivity data. 相似文献